PPMXL photometric study of two newly discovered open clusters

In this research we study the characteristics of two embedded young open star clusters which are newly discovered through the inspection of the infrared observations. These clusters and many others are hidden in the interstellar dust in the galactic disk from the optical previously surveys. For these clusters we determine the structural parameters (core radius limiting radius etc) and astrophysical parameters (reddening distance and age). We have selected two open star clusters; SAI 19 and SAI 23 the current work is the first study for these two clusters.